Relativistic self-gravitating gas in dynamical equilibrium
Alexander B. Kashuba

TL;DR
This paper derives a static, spherically symmetric solution to Einstein's equations for a relativistic self-gravitating gas in equilibrium, revealing a core with a universal fluid and a relativistic nucleus with singularity.
Contribution
It introduces a new exact solution describing a relativistic self-gravitating gas with a universal core and a relativistic nucleus, highlighting properties like incompressibility and particle bounce-back.
Findings
Development of a relativistic nucleus with focused gravitational fields
Universal perfect fluid description inside the nucleus
Presence of a point-like singularity at the center at the relativistic limit
Abstract
Static spherically symmetric solution of the Einstein's equations is found representing averaged properties of an infinite self-gravitating gas in the dynamical equilibrium. It depends upon three parameters: the core radius, the relativistic factor , defining the density and the mass, and one structural parameter. In the relativistic limit, , an open nucleus of focused gravitational fields develops with the size being a small fraction of the core radius whereas the outskirts of the self-gravitating gas remains non-relativistic. Inside the nucleus the self-gravitating gas is described by a universal perfect fluid with the relativistic one-dimensional equation of state. At , the space and time develops a point like singularity at the center. A characteristic property of the nucleus is incompressibility. New particles added to the self-gravitating gas bounce back into…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
